... m 4. free electron emission from neutron star surface small surface magnetic field ... c = 2 /P is angular velocity of neutron star, B is magnetic field strenght Particles ...
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Ссылки http://www.astro.spbu.ru/sobolev100/sites/default/files/barsukov_sobolev100_poster.pdf -- 587.9 Кб -- 25.03.2016 Похожие документы
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Ссылки http://www.astro.spbu.ru/Sobolev100/sites/default/files/ProgramFinal_0.pdf -- 313.0 Кб -- 28.09.2015 Похожие документы
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... a strong outburst, detected in all spectral regions from the -ray to the radio, which was explained by the interaction in a binary system, containing a B[e] supergiant and a compact degenerate companion (a neutron star or a black hole, see Robinson et al ...